High School Physics: Doppler Effect

In summary, the conversation is about finding the speed of sound using the Doppler frequency formula. The person is having trouble rearranging the formula and needs help. The correct formula is fd = (vw / (vw - vs)) fs. By multiplying both sides of the equation with (vw - vs), the person was able to solve for the speed of sound.
  • #1
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Homework Statement




An automobile is approaching you at a speed of 60.0 km/h and sounding its horn. The fundamental frequency of the horn sounds to you like 388 Hz. If the real fundamental frequency of the horn is 369 Hz, what is the speed of sound?


Homework Equations



Doppler Frequency = (speed of sound / (speed of sound - speed of source)) source frequency

fd = (vw/ vw - vs) fs

The Attempt at a Solution



What I'm having trouble with is rearranging the formula to solve for the speed of sound. Because there is two 'speed of sound' variables, you either end up dividing one by the other, and eliminating all variables; or subtracting one from the other, and (once again) eliminating all variables. As far as I can see, it's not possible?

Could someone help me out with rearranging this formula properly?

In case anyone's wondering, it's Grade 11 Physics.
 
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  • #2
You have the formula written down wrong.

You wrote:

fd = (vw/ vw - vs) fs

It's supposed to be:

fd = (vw / (vw - vs)) fs

Good luck!
 
  • #3
Try multiply both sides of the equation (when its written up correctly as Tusike noted) with vw-vs. The resulting equation should now be easier to solve for vw.
 
  • #4
Thanks alot! I got the correct answer, thanks to both of those pieces of advice.
 
  • #5


Dear student,

Thank you for your question. The Doppler effect is a phenomenon that is observed when there is relative motion between a source of sound and the observer. In this case, the source of sound is the automobile and the observer is you.

To solve for the speed of sound, we can use the formula you provided: fd = (vw/ vw - vs) fs

First, let's rearrange the formula to solve for the speed of sound:

vw = (fd * (vw - vs)) / fs

Now, we can substitute the given values into the formula:

vw = (388 Hz * (60.0 km/h - 0 km/h)) / 369 Hz

vw = 62.6 km/h

This is the velocity of the wave relative to the observer. Since the observer is stationary, this is also the speed of sound.

Therefore, the speed of sound is 62.6 km/h.

I hope this helps. Keep up the good work in your physics studies!

Best,

Scientist
 

Related to High School Physics: Doppler Effect

What is the Doppler Effect?

The Doppler Effect is the change in frequency or wavelength of a wave in relation to an observer's motion. It occurs when there is relative motion between the source of the wave and the observer.

How does the Doppler Effect apply to high school physics?

The Doppler Effect is an important concept in high school physics as it explains the change in frequency of sound waves, light waves, or any other type of wave, due to the relative motion between the source and the observer. It is often used in topics such as sound waves, electromagnetic radiation, and astronomy.

How is the Doppler Effect calculated?

The Doppler Effect can be calculated using the formula: f' = f(v ± vr)/(v ± vs), where f' is the observed frequency, f is the original frequency, v is the speed of the wave, vr is the velocity of the receiver (observer), and vs is the velocity of the source. This formula takes into account the relative motion between the source and the observer.

What are some real-life examples of the Doppler Effect?

The Doppler Effect can be observed in everyday life. For example, the change in pitch of a siren as an ambulance or police car passes by, the change in frequency of a train's whistle as it approaches and passes by, and the change in color of a star's light as it moves towards or away from Earth are all examples of the Doppler Effect in action.

How does the Doppler Effect affect our understanding of the universe?

The Doppler Effect plays a crucial role in our understanding of the universe. It allows us to measure the movement and velocity of celestial objects, such as stars and galaxies, by analyzing the change in the frequency of the light they emit. This information helps us to understand the size, age, and evolution of the universe.

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